摘要
为了分析食双星AK Cam和BW Del的轨道周期变化,本文从数据库O-C Gateway中收集了已发表的食双星AK Cam和BW Del的极小时刻。通过线性拟合,得到了这两颗食双星的线性历元公式和线性拟合的残差,并发现AK Cam和BW Del的O-C曲线都存在开口向上的抛物线变化。通过利用最小二乘法,获得了AK Cam和BW Del轨道周期增加率分别为3.27(±0.03)×10^-7天/年和1.14(±0.01)×10^-6天/年。对于AK Cam和BW Del,其轨道周期变化都很可能是由星风带走恒星物质导致。
The published minimum times for two eclipsing binaries of AK Cam and BW Del from O-C Gateway database were used to analyze their orbital period variation. Using linear fitting,the linear ephemeris and residuals of linear fitting were derived and the upward parabola variations of O-C curves for the two binaries were found. By using least squares,the growth rates of orbital period for AK Cam and BW Del were 3.27( ±0.03) ×10^-7 d/y and 1.14( ±0.01) ×10-6 d/y respectively. Results show that the orbital period variations of AK Cam and BW Del could be affected due to the mass carried off by the solar wind.
作者
岳强
朱仲忠
YUE Qiang;ZHU Zhongzhong(Department of Physics and Astronomy, College of Physics, Guizhou University, Guiyang 550025, China)
出处
《贵州大学学报(自然科学版)》
2019年第4期37-42,共6页
Journal of Guizhou University:Natural Sciences
基金
国家自然科学基金项目资助(U1431114,U1631236)
关键词
食双星AK
Cam
BW
DEL
周期变化
物理机制
eclipsing binaries of AK Cam and BW Del
periodic variation
physical mechanism